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Dive into the research topics where X. T. Huang is active.

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Featured researches published by X. T. Huang.


Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1999

Detection of scintillation light in coincidence with ionizing tracks in a liquid argon time projection chamber

P. Cennini; J.-P. Revol; C. Rubbia; F. Sergiampietri; A. Bueno; M. Campanelli; P Goudsmit; A. Rubbia; L. Periale; S. Suzuki; C. Chen; Y. X. Chen; K. He; X. T. Huang; Z. Li; F. Lu; J. Ma; G. Xu; Z. Xu; C. C. Zhang; Qingmin Zhang; S.C. Zheng; F. Cavanna; D. Mazza; G. Piano Mortari; S. Petrera; C. Rossi; G. Mannocchi; P. Picchi; F. Arneodo

A system to detect light from liquid argon scintillation has been implemented in a small, ICARUS-like, liquid argon time projection chamber. The system, which uses a VUV-sensitive photomultiplier to collect the light, has recorded many ionizing tracks from cosmic-rays in coincidence with scintillation signals. Our measurements demonstrate that scintillation light detection can provide an effective method for absolute time measurement of events and eventually a useful trigger signal


Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2000

Study of solar neutrinos with the 600 t liquid argon ICARUS detector

F. Arneodo; A. Badertscher; S Baibussinov; P. Benetti; A.Borio di Tigliole; R. Brunetti; A. Bueno; E. Calligarich; M. Campanelli; C. Carpanese; D. Cavalli; F. Cavanna; P. Cennini; S. Centro; A. Cesana; C. Chen; Y. X. Chen; D. Cline; I. De Mitri; R. Dolfini; A. Ferrari; A. Gigli Berzolari; P Goudsmit; K. He; X. T. Huang; Z. Li; F. Lu; J. Ma; G. Mannocchi; M Maris

Abstract The ICARUS time projection chamber can yield sound information on 8 B solar neutrinos. Owing to the high-energy resolution and the good capability of event reconstruction it can make a contribution to our understanding of neutrino intensities and their energy spectrum. Moreover, the MSW oscillation probability for sterile and active neutrinos can be well studied because both elastic scattering by electrons and absorption reaction on argon nuclei can be measured independently. The main problem in detecting the low-energy neutrino interactions arises from the environmental radioactivity. In the present work we study by Monte Carlo simulation the topology and the rates of the events, induced by neutrinos and background neutrons, in a 470 t (fiducial mass) liquid-argon TPC detector. For neutrino interactions we use the standard solar model BP98 and the recent experimental confirmation of the shell model computation of absorption cross section. The noise is estimated from new data on natural neutron background, collected in the hall C of the Gran Sasso laboratory. It is confirmed that, with a relatively modest neutron shielding and particular off-line event triggers, the weight of spurious events can be made to have little influence on the ICARUS solar neutrino measurement. Indeed, we expect 6 (26) background events per year in the 212 (759) elastic scattering (absorption reaction) sample.


Physical Review D | 2013

Study of

M. Ablikim; M. N. Achasov; O. Albayrak; D. J. Ambrose; F. F. An; Q. An; J. Z. Bai; R. Baldini Ferroli; Y. Ban; J. Becker; J. V. Bennett; M. Bertani; J. M. Bian; E. Boger; O. Bondarenko; I. Boyko; R. A. Briere; V. Bytev; H. Cai; X. Cai; O. Cakir; A. Calcaterra; G. F. Cao; S. A. Cetin; J. F. Chang; G. A. Chelkov; G. Chen; H. S. Chen; J. C. Chen; M. L. Chen

The decay


Nuclear Physics B - Proceedings Supplements | 2000

J/\psi \rightarrow \omega p \bar{p}

C. Vignoli; F. Arneodo; A. Badertscher; E. Barbieri; P. Benetti; A.Borio di Tigliole; R. Brunetti; A. Bueno; E. Calligarich; M. Campanelli; F. Carli; C. Carpanese; D. Cavalli; F. Cavanna; P. Cennini; S. Centro; A. Cesana; C. Chen; Y. X. Chen; C. Cinquini; D. Cline; I. De Mitri; R. Dolfini; D. Favaretto; A. Ferrari; A. Gigli Berzolari; P Goudsmit; K. He; X. T. Huang; Z. Li

J/\psi \rightarrow \omega p \bar{p}


Physical Review D | 2013

at BESIII

M. Ablikim; M. N. Achasov; X. C. Ai; O. Albayrak; D. J. Ambrose; F. F. An; Q. An; J. Z. Bai; R. Baldini Ferroli; Y. Ban; J. V. Bennett; M. Bertani; J. M. Bian; E. Boger; O. Bondarenko; I. Boyko; S. Braun; R. A. Briere; H. Cai; X. Cai; O. Cakir; A. Calcaterra; G. F. Cao; S. A. Cetin; J. F. Chang; G. A. Chelkov; G. Chen; H. S. Chen; J. C. Chen; M. L. Chen

has been studied, using


Physical Review D | 2013

ICARUS 600 ton: A status report

M. Ablikim; M. N. Achasov; O. Albayrak; D. J. Ambrose; F. F. An; Q. An; J. Z. Bai; R. Baldini Ferroli; Y. Ban; J. Becker; J. V. Bennett; N. Berger; M. Bertani; J. M. Bian; E. Boger; O. Bondarenko; I. Boyko; R. A. Briere; V. Bytev; H. Cai; X. Cai; O. Cakir; A. Calcaterra; G. F. Cao; S. A. Cetin; J. F. Chang; G. A. Chelkov; G. Chen; H. S. Chen; J. C. Chen

225.3\times 10^{6}


Physical Review Letters | 2012

Search for the

O. Bondarenko; J. C. Chen; Min Chen; J. P. Dai; Y. Gao; J. S. Huang; X. T. Huang; L. K. Jia; S. L. Jin; N. Kalantar-Nayestanaki; M. Kavatsyuk; J. S. Lange; F. Y. Li; Guihua Li; Haibo B. Li; N. B. Li; S. L. Li; Hao Liang; Y. T. Liang; G. R. Liao; C. L. Liu; C. X. Liu; C. Y. Liu; K. Liu; K. Y. Liu; H. Loehner; J. G. Lu; X. L. Luo; C. L. Ma; J. G. Messchendorp


Physical Review D | 2011

\eta_c(2S)/h_c\to p\bar{p}

M. Ablikim; M. N. Achasov; O. Bondarenko; J. C. Chen; M. L. Chen; J. P. Dai; Y. Gao; J. S. Huang; X. T. Huang; L. K. Jia; S. Jin; M. Kavatsyuk; J. S. Lange; F. Y. Li; G. Li; H. B. Li; N. B. Li; Hao Liang; Y. T. Liang; G. R. Liao; C. L. Liu; C. X. Liu; C. Y. Liu; G. C. Liu; K. Liu; K. Y. Liu; Z. Q. Liu; H. Loehner; J. G. Lu; X. L. Luo

J/\psi


Physical Review Letters | 2005

decays and measurements of the

M. Ablikim; J. Z. Bai; Y. Ban; J.G. Bian; X. Cai; H.F. Chen; H. S. Chen; H.X. Chen; J. C. Chen; Jin Chen; Y. B. Chen; S.P. Chi; Y. P. Chu; X.Z. Cui; Y.S. Dai; Z. Y. Deng; L. Y. Dong; Q.F. Dong; S. X. Du; Z.Z. Du; J. Fang; S. S. Fang; C. D. Fu; C.S. Gao; Y. Gao; S.D. Gu; Y. T. Gu; Y. Guo; Y. Q. Guo; Z. J. Guo

events accumulated at BESIII. No significant enhancement near the


Physical Review Letters | 2008

\chi_{cJ}\to p\bar{p}

M. Ablikim; J. Z. Bai; Y. Bai; Y. Ban; X. Cai; H.F. Chen; H. S. Chen; H.X. Chen; J. C. Chen; Jin Chen; X. Chen; Y. B. Chen; Y. P. Chu; Y.S. Dai; Z. Y. Deng; S. X. Du; J. Fang; C. D. Fu; C.S. Gao; Y. Gao; S.D. Gu; Y. T. Gu; Y. Guo; Z. J. Guo; F. A. Harris; K. L. He; M. He; Y. K. Heng; J. Hou; H. M. Hu

p\bar{p}

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J. C. Chen

Chinese Academy of Sciences

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M. Ablikim

Chinese Academy of Sciences

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J. Z. Bai

Chinese Academy of Sciences

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X. Cai

Chinese Academy of Sciences

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Y. Gao

Tsinghua University

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Y. B. Chen

Chinese Academy of Sciences

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C. D. Fu

Chinese Academy of Sciences

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